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SUMMARY:External Colloquium | Lyndsay Fletcher (U. of Glasgow)
DTSTART:20250410T120000Z
DTEND:20250410T140000Z
DTSTAMP:20260417T080900Z
UID:www.aip.de-2022
CATEGORIES:Scientific
CATEGORIES:Generic Event
CATEGORIES:Public
CONTACT:Julián Alvarado-Gómez <julian.alvarado-gomez@aip.de>
DESCRIPTION:The fine scales of solar chromospheric flaresA solar flare is 
 an intense but short-lived release of energy from the Sun&#x27\;s magnetic
 ally-dominated atmosphere\, resulting in the acceleration of non-thermal p
 articles\, plasma heating\, and radiation across the entire electromagneti
 c spectrum. Most energy released is radiated by the solar chromosphere\, g
 iving rise to bright\, highly structured &#x27\;footpoints&#x27\; and &#x2
 7\;ribbons&#x27\; of chromospheric emission. The big picture of a solar fl
 are\, and the significance of flare ribbons in the global reconnection sce
 nario\, is well established\, but high-resolution observations show fine s
 patial\, temporal and spectral structure which can be probed to further ex
 plore flare physics. In this talk I will overview the basic framework of a
  solar flare and its development in the solar chromosphere\, highlighting 
 some examples of how fine scales are being used to investigate energy rele
 ase and transport. I will focus on results from the IRIS spacecraft in the
  UV\, and a newly-opened window on flares in the mid-infrared.\n
LOCATION:Maria Margaretha Kirch Haus Konferenzraum
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